Isotope ratios can be measured in presolar SiC grains from ancient asymptotic giant branch
(AGB) stars at permil-level (0.1%) precision. Such precise grain data permit derivation of …

Recent models for evolved low-mass stars (with M≲ 3 M⊙), undergoing the asymptotic giant
branch (AGB) phase assume that magnetic flux-tube buoyancy drives the formation of 13 C …

We present post-process neutron-capture computations for Asymptotic Giant Branch (AGB)
stars of 1.5–3 M⊙ and metallicities− 1.3≤[Fe/H]≤ 0.1. The reference stellar models are …

The competing $^{22} $ Ne ($\alpha,\gamma $) $^{26} $ Mg and $^{22} $ Ne ($\alpha, n $)
$^{25} $ Mg reactions control the production of neutrons for the weak $ s $-process in …

Asymptotic giant branch (AGB) stars are considered to be among the most significant
contributors to the fluorine budget in our Galaxy. While observations and theory agree at …

Low-mass asymptotic giant branch stars are among the most important polluters of the
interstellar medium. In their interiors, the main component (A≳ 90) of the slow neutron …

Asymptotic Giant Branch (AGB) stars are among the most important astrophysical sites
influencing the nucleosynthesis and the chemical abundances in the Universe. From a pure …

Stardust grains that originated in ancient stars and supernovae are recovered from
meteorites and carry the detailed composition of their astronomical sites of origin. We …

We compare updated Torino postprocessing asymptotic giant branch (AGB) nucleosynthesis
model calculations with isotopic compositions of mainstream SiC dust grains from low-mass …

We present new fluorine abundance measurements for a sample of carbon-rich asymptotic
giant branch (AGB) stars and two other metal-poor evolved stars of Ba/CH types. The …